Cosmological relevance of scaling solutions: a recipe for quintessential inflation
DOI10.1007/S10714-022-02969-6OpenAlexW4291824397MaRDI QIDQ2675170
Publication date: 20 September 2022
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-022-02969-6
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Numerical computation of matrix norms, conditioning, scaling (65F35) Classical and relativistic thermodynamics (80A10) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Dark matter and dark energy (83C56)
Related Items (2)
Cites Work
- Quintessential inflation from a variable cosmological constant in a 5D vacuum
- Steep inflation followed by Born-Infeld reheating
- Quintessential enhancement of dark matter abundance
- Sub-horizon perturbation behavior in extended quintessence
- On the potentials yielding cosmological scaling solutions
- Warm quintessential inflation
- A new type of isotropic cosmological models without singularity
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Cosmological backgrounds of gravitational waves
- DYNAMICS OF DARK ENERGY
- Reconstructing a model of quintessential inflation
- Inflation and transition to a slowly accelerating phase from SSB of scale invariance
- Unification of inflation and dark energyà laquintessential inflation
- Inflationary universe: A possible solution to the horizon and flatness problems
- Inflation, braneworlds and quintessence
This page was built for publication: Cosmological relevance of scaling solutions: a recipe for quintessential inflation